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Recently, we proposed an enhancement of the Regge-Wheeler-Zerilli formalismfor first-order perturbations about a Schwarzschild background that includesfirst-order corrections due to the background black-hole spin. Using thisformalism, we investigate gravitational wave recoil effects from a spinningblack-hole binary system analytically. This allows us to better understand theorigin of the large recoils observed in full numerical simulation of spinningblack hole binaries.

Perturbative effects of spinning black holes with applications to recoil velocities